Nucleosynthesis of Heavy Elements in Neutrino-Driven Winds and Neutron-Star Mergers
APA
Arcones, A. (2011). Nucleosynthesis of Heavy Elements in Neutrino-Driven Winds and Neutron-Star Mergers. Perimeter Institute. https://pirsa.org/11060027
MLA
Arcones, Almudena. Nucleosynthesis of Heavy Elements in Neutrino-Driven Winds and Neutron-Star Mergers. Perimeter Institute, Jun. 22, 2011, https://pirsa.org/11060027
BibTex
@misc{ pirsa_PIRSA:11060027, doi = {10.48660/11060027}, url = {https://pirsa.org/11060027}, author = {Arcones, Almudena}, keywords = {Particle Physics}, language = {en}, title = {Nucleosynthesis of Heavy Elements in Neutrino-Driven Winds and Neutron-Star Mergers}, publisher = {Perimeter Institute}, year = {2011}, month = {jun}, note = {PIRSA:11060027 see, \url{https://pirsa.org}} }
Universität Basel
Talk Type
Subject
Abstract
The energy generated by the r-process can impact the dynamics of neutron star mergers. Solving a full r-process network coupled with the hydrodynamics becomes the necessary but it is computational very expensive. We have developed a simple model that can be implemented into hydrodynamic simulations and gives a very good estimate of the r-process heating.